Storage |
Field name |
Units |
Description |
Default |
All |
Provenance field name |
File |
HDU |
A |
cz |
None |
z of Normal unit vector in J2000 |
False |
True |
CZ |
specObj-dr17 |
1 |
A |
elodie_z |
None |
Redshift fit to ELODIE star |
False |
True |
ELODIE_Z |
specObj-dr17 |
1 |
A |
specsegue |
None |
Set to 1 for primary SDSS SEGUE program observation of object (including SEGUE-1 and SEGUE-2), 0 otherwise |
False |
True |
SPECSEGUE |
specObj-dr17 |
1 |
A |
anyandmask |
None |
For each bit, records whether any pixel in the spectrum has that bit set in its ANDMASK |
False |
True |
ANYANDMASK |
specObj-dr17 |
1 |
A |
elodie_rchi2 |
None |
Reduced chi-squared of fit to best ELODIE star |
False |
True |
ELODIE_RCHI2 |
specObj-dr17 |
1 |
A |
nturnoff |
None |
Number of stars used for SNTURNOFF determination |
False |
True |
NTURNOFF |
specObj-dr17 |
1 |
A |
vdispdof |
None |
Number of degrees of freedom in velocity dispersion fit |
False |
True |
VDISPDOF |
specObj-dr17 |
1 |
A |
specsegue1 |
None |
Set to 1 for primary SDSS SEGUE-1 program observation of object, 0 otherwise |
False |
True |
SPECSEGUE1 |
specObj-dr17 |
1 |
A |
elodie_z_err |
None |
Error in redshift fit to ELODIE star |
False |
True |
ELODIE_Z_ERR |
specObj-dr17 |
1 |
A |
lambda_eff |
AA |
Effective wavelength drilling position was optimized for |
False |
True |
LAMBDA_EFF |
specObj-dr17 |
1 |
A |
eboss_target1 |
None |
eBOSS, TDSS and SPIDERS target selection flags for main eBOSS survey |
False |
True |
EBOSS_TARGET1 |
specObj-dr17 |
1 |
A |
snturnoff |
None |
Signal to noise measure for MS turnoff stars on plate (-9999 if not appropriate) |
False |
True |
SNTURNOFF |
specObj-dr17 |
1 |
A |
spec1_i |
None |
Signal-to-noise squared for spectrograph #1, at i=19.90 for SDSS spectrograph spectra, i=20.20 for BOSS spectrograph spectra |
False |
True |
SPEC1_I |
specObj-dr17 |
1 |
A |
specsegue2 |
None |
Set to 1 for primary SDSS SEGUE-2 program observation of object, 0 otherwise |
False |
True |
SPECSEGUE2 |
specObj-dr17 |
1 |
A |
spectrographid |
None |
Which spectrograph (1 or 2) |
False |
True |
SPECTROGRAPHID |
specObj-dr17 |
1 |
A |
objid |
None |
SDSS photometric object identification numbers (RUN, RERUN, CAMCOL, FIELD, ID) |
False |
True |
OBJID |
specObj-dr17 |
1 |
A |
z_conf_person |
None |
Visual-inspection confidence (0=not inspected or no confidence, 1,2=low confidence, 3,4=high confidence) |
False |
True |
Z_CONF_PERSON |
specObj-dr17 |
1 |
A |
z_person |
None |
Visual-inspection redshift |
False |
True |
Z_PERSON |
specObj-dr17 |
1 |
A |
elodie_feh |
None |
Metallicity [Fe/H] of ELODIE star |
False |
True |
ELODIE_FEH |
specObj-dr17 |
1 |
A |
spectrosynflux |
nanomaggy |
Best-fit template spectrum projected onto ugriz filters |
False |
True |
SPECTROSYNFLUX |
specObj-dr17 |
1 |
A |
spec2_r |
None |
Signal-to-noise squared for spectrograph #2, at r=20.25 for SDSS spectrograph spectra, r=20.20 for BOSS spectrograph spectra |
False |
True |
SPEC2_R |
specObj-dr17 |
1 |
A |
sourcetype |
None |
String expressing type of source (similar to OBJTYPE in DR8 and earlier) |
False |
True |
SOURCETYPE |
specObj-dr17 |
1 |
A |
plate |
None |
Plate number (each plate corresponds to an actual plug plate) |
False |
True |
PLATE |
specObj-dr17 |
1 |
A |
chi68p |
None |
68-th percentile value of abs(chi) of the best-fit synthetic spectrum to the actual spectrum (around 1.0 for a good fit) |
False |
True |
CHI68P |
specObj-dr17 |
1 |
A |
fluxobjid |
None |
Unique database ID of flux-based photometric match based on RUN, RERUN, CAMCOl, FIELD, ID (same as SkyServer version) |
False |
True |
FLUXOBJID |
specObj-dr17 |
1 |
A |
spec2_i |
None |
Signal-to-noise squared for spectrograph #2, at i=19.90 for SDSS spectrograph spectra, i=20.20 for BOSS spectrograph spectra |
False |
True |
SPEC2_I |
specObj-dr17 |
1 |
A |
eboss_target_id |
None |
EBOSS unique target identifier for every spectroscopic target |
False |
True |
EBOSS_TARGET_ID |
specObj-dr17 |
1 |
A |
segue2_target2 |
None |
Secondary (calibration) target flags for SEGUE-2 targets |
False |
True |
SEGUE2_TARGET2 |
specObj-dr17 |
1 |
A |
fracnsighi |
None |
Fraction of pixels high by more than N sigma relative to best-fit (for 1,2,..,10 sigma) |
False |
True |
FRACNSIGHI |
specObj-dr17 |
1 |
A |
elodie_logg |
None |
log10(gravity) of ELODIE star |
False |
True |
ELODIE_LOGG |
specObj-dr17 |
1 |
A |
theta |
None |
Template coefficients of best fit |
False |
True |
THETA |
specObj-dr17 |
1 |
A |
firstrelease |
None |
Name of first release this PLATE, MJD, FIBERID, RUN2D was associated with |
False |
True |
FIRSTRELEASE |
specObj-dr17 |
1 |
A |
elodie_dof |
None |
Degrees of freedom in fit to best ELODIE star |
False |
True |
ELODIE_DOF |
specObj-dr17 |
1 |
A |
anyormask |
None |
For each bit, records whether any pixel in the spectrum has that bit set in its ORMASK |
False |
True |
ANYORMASK |
specObj-dr17 |
1 |
A |
sn_median_all |
None |
Median signal-to-noise per pixel across full spectrum |
False |
True |
SN_MEDIAN_ALL |
specObj-dr17 |
1 |
A |
primtarget |
None |
Target selection information at plate design, primary science selection (for backwards compatibility) |
False |
True |
PRIMTARGET |
specObj-dr17 |
1 |
A |
run2d |
None |
Spectroscopic 2D reduction (extraction of spectra) name |
False |
True |
RUN2D |
specObj-dr17 |
1 |
A |
tile |
None |
Tile number (each tile can have several plates drilled for it) |
False |
True |
TILE |
specObj-dr17 |
1 |
A |
thing_id |
None |
Resolve THING_ID in SDSS imaging for best positional match |
False |
True |
THING_ID |
specObj-dr17 |
1 |
A |
elodie_object |
None |
Star name for ELODIE star |
False |
True |
ELODIE_OBJECT |
specObj-dr17 |
1 |
A |
special_target2 |
None |
Secondary (calibration) target flags for SDSS-I and SDSS-II special program targets |
False |
True |
SPECIAL_TARGET2 |
specObj-dr17 |
1 |
A |
vdispz_err |
None |
Error in redshift associated with best-fit velocity dispersion |
False |
True |
VDISPZ_ERR |
specObj-dr17 |
1 |
A |
calibflux |
nanomaggy |
ugriz fluxes used for calibrations |
False |
True |
CALIBFLUX |
specObj-dr17 |
1 |
A |
vdisp_err |
km s-1 |
Error in velocity dispersion |
False |
True |
VDISP_ERR |
specObj-dr17 |
1 |
A |
segue1_target2 |
None |
Primary (science) target flags for SEGUE-1 targets |
False |
True |
SEGUE1_TARGET2 |
specObj-dr17 |
1 |
A |
nspecobs |
None |
Number of spectroscopic observations of this source |
False |
True |
NSPECOBS |
specObj-dr17 |
1 |
A |
boss_target1 |
None |
Primary (science) target flags for BOSS targets |
False |
True |
BOSS_TARGET1 |
specObj-dr17 |
1 |
A |
wcoverage |
None |
Coverage in wavelength, in units of log10 wavelength |
False |
True |
WCOVERAGE |
specObj-dr17 |
1 |
A |
speclegacy |
None |
Set to 1 for primary SDSS Legacy program observation of object, 0 otherwise |
False |
True |
SPECLEGACY |
specObj-dr17 |
1 |
A |
xfocal |
mm |
Hole position on plate (+X = +RA) |
False |
True |
XFOCAL |
specObj-dr17 |
1 |
A |
spectroskyflux |
nanomaggy |
Sky flux in each of the ugriz imaging filters |
False |
True |
SPECTROSKYFLUX |
specObj-dr17 |
1 |
A |
specboss |
None |
Set to 1 for primary BOSS spectrograph observation of object, 0 otherwise |
False |
True |
SPECBOSS |
specObj-dr17 |
1 |
A |
subclass |
None |
Best spectroscopic subclassification |
False |
True |
SUBCLASS |
specObj-dr17 |
1 |
A |
comments_person |
None |
Visual-inspection comments |
False |
True |
COMMENTS_PERSON |
specObj-dr17 |
1 |
A |
sectarget |
None |
Deprecated version of secondary (calibration) target flags (meanings highly overloaded) |
False |
True |
SECTARGET |
specObj-dr17 |
1 |
A |
spectroflux_ivar |
nanomaggy-2 |
Inverse variance of spectrum projected onto ugriz filters |
False |
True |
SPECTROFLUX_IVAR |
specObj-dr17 |
1 |
A |
targetobjid |
None |
Unique database ID of targeting object based on RUN, RERUN, CAMCOl, FIELD, ID (same as SkyServer version) |
False |
True |
TARGETOBJID |
specObj-dr17 |
1 |
A |
tcolumn |
None |
Columns of template files that correspond to each template |
False |
True |
TCOLUMN |
specObj-dr17 |
1 |
A |
spectroflux |
nanomaggy |
Spectrum projected onto ugriz filters |
False |
True |
SPECTROFLUX |
specObj-dr17 |
1 |
A |
rchi2 |
None |
Reduced chi-squared of best fit |
False |
True |
RCHI2 |
specObj-dr17 |
1 |
A |
fracnsiglo |
None |
Fraction of pixels low by more than N sigma relative to best-fit (for 1,2,..,10 sigma) |
False |
True |
FRACNSIGLO |
specObj-dr17 |
1 |
A |
spectrosynflux_ivar |
nanomaggy-2 |
Inverse variance of best-fit template spectrum projected onto ugriz filters |
False |
True |
SPECTROSYNFLUX_IVAR |
specObj-dr17 |
1 |
A |
class_person |
None |
Visual-inspection classification (0=not inspected or unknown, 1=star, 2=narrow emission-line galaxy, 3=QSO, 4=galaxy) |
False |
True |
CLASS_PERSON |
specObj-dr17 |
1 |
A |
ancillary_target1 |
None |
BOSS ancillary science target selection information at plate design |
False |
True |
ANCILLARY_TARGET1 |
specObj-dr17 |
1 |
A |
boss_specobj_id |
None |
Identification number internal to BOSS for SPECBOSS=1 objects |
False |
True |
BOSS_SPECOBJ_ID |
specObj-dr17 |
1 |
A |
survey |
None |
Survey name |
False |
True |
SURVEY |
specObj-dr17 |
1 |
A |
platerun |
None |
Drilling run that this plate was drilled in |
False |
True |
PLATERUN |
specObj-dr17 |
1 |
A |
targettype |
None |
General type of target (SCIENCE, STANDARD, or SKY) |
False |
True |
TARGETTYPE |
specObj-dr17 |
1 |
A |
designid |
None |
Design identification number for plate |
False |
True |
DESIGNID |
specObj-dr17 |
1 |
A |
segue2_target1 |
None |
Primary (science) target flags for SEGUE-2 targets |
False |
True |
SEGUE2_TARGET1 |
specObj-dr17 |
1 |
A |
legacy_target2 |
None |
Secondary (calibration) target flags for SDSS-I and SDSS-II Legacy survey |
False |
True |
LEGACY_TARGET2 |
specObj-dr17 |
1 |
A |
ancillary_target2 |
None |
BOSS ancillary target selection information at plate design |
False |
True |
ANCILLARY_TARGET2 |
specObj-dr17 |
1 |
A |
platesn2 |
None |
Overall signal-to-noise-squared measure for plate (only for SDSS spectrograph plates) |
False |
True |
PLATESN2 |
specObj-dr17 |
1 |
A |
class_noqso |
None |
Spectroscopic classification for Z_NOQSO redshift |
False |
True |
CLASS_NOQSO |
specObj-dr17 |
1 |
A |
chunk |
None |
Name of tiling chunk that this spectrum was tiled in (boss1, boss2, etc), important for tracking large-scale structure samples |
False |
True |
CHUNK |
specObj-dr17 |
1 |
A |
bluefiber |
None |
Set to 1 if this hole was designated a blue fiber, 0 if designated a red fiber (high redshift LRGs are preferentially in red fibers) |
False |
True |
BLUEFIBER |
specObj-dr17 |
1 |
A |
elodie_teff |
Kelvin |
Effective temperature of ELODIE star |
False |
True |
ELODIE_TEFF |
specObj-dr17 |
1 |
A |
thing_id_targeting |
None |
Resolve THING_ID in SDSS imaging for targeted object |
False |
True |
THING_ID_TARGETING |
specObj-dr17 |
1 |
A |
elodie_sptype |
None |
ELODIE star spectral type |
False |
True |
ELODIE_SPTYPE |
specObj-dr17 |
1 |
A |
spec2_g |
None |
Signal-to-noise squared for spectrograph #2, at g=20.20 for SDSS spectrograph spectra, g=21.20 for BOSS spectrograph spectra |
False |
True |
SPEC2_G |
specObj-dr17 |
1 |
A |
vdispz |
None |
Redshift associated with best-fit velocity dispersion |
False |
True |
VDISPZ |
specObj-dr17 |
1 |
A |
marvels_target2 |
None |
Secondary (calibration) target flags for MARVELS targets |
False |
True |
MARVELS_TARGET2 |
specObj-dr17 |
1 |
A |
fracnsigma |
None |
Fraction of pixels deviant by more than N sigma relative to best-fit (for 1,2,..,10 sigma) |
False |
True |
FRACNSIGMA |
specObj-dr17 |
1 |
A |
spec1_r |
None |
Signal-to-noise squared for spectrograph #1, at r=20.25 for SDSS spectrograph spectra, r=20.20 for BOSS spectrograph spectra |
False |
True |
SPEC1_R |
specObj-dr17 |
1 |
A |
zwarning_noqso |
None |
Warnings in z_noqso redshift (BOSS spectra only) |
False |
True |
ZWARNING_NOQSO |
specObj-dr17 |
1 |
A |
npoly |
None |
Number of polynomial terms in fit |
False |
True |
NPOLY |
specObj-dr17 |
1 |
A |
run1d |
None |
Spectroscopic 1D reduction (redshift and classification) name |
False |
True |
RUN1D |
specObj-dr17 |
1 |
A |
eboss_target2 |
None |
eBOSS, TDSS and SPIDERS target selection flags for main eBOSS survey |
False |
True |
EBOSS_TARGET2 |
specObj-dr17 |
1 |
A |
rchi2diff_noqso |
None |
Difference in reduced chi-squared between best and second best fit for Z_NOQSO redshift |
False |
True |
RCHI2DIFF_NOQSO |
specObj-dr17 |
1 |
A |
subclass_noqso |
None |
Spectroscopic subclassification for Z_NOQSO redshift |
False |
True |
SUBCLASS_NOQSO |
specObj-dr17 |
1 |
A |
dof |
None |
Number of degrees of freedom in best fit |
False |
True |
DOF |
specObj-dr17 |
1 |
A |
z_err_noqso |
None |
Error in Z_NOQSO redshift |
False |
True |
Z_ERR_NOQSO |
specObj-dr17 |
1 |
A |
fiberid |
None |
Fiber number |
False |
True |
FIBERID |
specObj-dr17 |
1 |
A |
cx |
None |
x of Normal unit vector in J2000 |
False |
True |
CX |
specObj-dr17 |
1 |
A |
mjd |
days |
Modified Julian Day of observation |
False |
True |
MJD |
specObj-dr17 |
1 |
A |
specsdss |
None |
Set to 1 for primary SDSS spectrograph observation of object, 0 otherwise |
False |
True |
SPECSDSS |
specObj-dr17 |
1 |
A |
tfile |
None |
File that best fit template comes from in idlspec2d product |
False |
True |
TFILE |
specObj-dr17 |
1 |
A |
calibflux_ivar |
nanomaggy-2 |
Inverse variances of ugriz fluxes used for calibrations |
False |
True |
CALIBFLUX_IVAR |
specObj-dr17 |
1 |
A |
elodie_z_modelerr |
None |
Standard deviation in redshift among the 12 best-fit ELODIE stars |
False |
True |
ELODIE_Z_MODELERR |
specObj-dr17 |
1 |
A |
special_target1 |
None |
Primary (science) target flags for SDSS-I and SDSS-II special program targets |
False |
True |
SPECIAL_TARGET1 |
specObj-dr17 |
1 |
A |
vdispchi2 |
None |
Chi-squared for best-fit velocity dispersion |
False |
True |
VDISPCHI2 |
specObj-dr17 |
1 |
A |
vdisp |
km s-1 |
Velocity dispersion |
False |
True |
VDISP |
specObj-dr17 |
1 |
A |
platequality |
None |
Final quality of plate this spectrum came from (good, marginal, or bad) |
False |
True |
PLATEQUALITY |
specObj-dr17 |
1 |
A |
spec1_g |
None |
Signal-to-noise squared for spectrograph #1, at g=20.20 for SDSS spectrograph spectra, g=21.20 for BOSS spectrograph spectra |
False |
True |
SPEC1_G |
specObj-dr17 |
1 |
A |
cy |
None |
y of Normal unit vector in J2000 |
False |
True |
CY |
specObj-dr17 |
1 |
A |
segue1_target1 |
None |
Primary (science) target flags for SEGUE-1 targets |
False |
True |
SEGUE1_TARGET1 |
specObj-dr17 |
1 |
A |
plateid |
None |
Unique database ID of plate based on PLATE, MJD, RUN2D (same as SkyServer version) |
False |
True |
PLATEID |
specObj-dr17 |
1 |
A |
deredsn2 |
None |
Dereddened overall signal-to-noise-squared measure for plate (only for BOSS spectrograph plates) |
False |
True |
DEREDSN2 |
specObj-dr17 |
1 |
A |
marvels_target1 |
None |
Primary (science) target flags for MARVELS targets |
False |
True |
MARVELS_TARGET1 |
specObj-dr17 |
1 |
A |
elodie_bv |
mag |
(B-V) color index for ELODIE star |
False |
True |
ELODIE_BV |
specObj-dr17 |
1 |
A |
legacy_target1 |
None |
Primary (science) target flags for SDSS-I and SDSS-II Legacy survey |
False |
True |
LEGACY_TARGET1 |
specObj-dr17 |
1 |
A |
rchi2diff |
None |
Difference in reduced chi-squared between best and second best fit |
False |
True |
RCHI2DIFF |
specObj-dr17 |
1 |
A |
sn_median |
None |
Median signal-to-noise per pixel within each of the ugriz bandpasses |
False |
True |
SN_MEDIAN |
specObj-dr17 |
1 |
A |
zoffset |
micron |
Washer thickness used for backstopping BOSS quasar targets, so they are closer to 4000 Angstrom focal plan |
False |
True |
ZOFFSET |
specObj-dr17 |
1 |
A |
vdispnpix |
None |
Number of pixels overlapping the templates used in the velocity dispersion fit |
False |
True |
VDISPNPIX |
specObj-dr17 |
1 |
A |
boss_target2 |
None |
Always set to zero (placeholder for BOSS target flags never used) |
False |
True |
BOSS_TARGET2 |
specObj-dr17 |
1 |
A |
yfocal |
mm |
Hole position on plate (+Y = +DEC) |
False |
True |
YFOCAL |
specObj-dr17 |
1 |
A |
elodie_filename |
None |
File name for best-fit ELODIE star |
False |
True |
ELODIE_FILENAME |
specObj-dr17 |
1 |
A |
programname |
None |
Program within each survey that the plate was part of |
False |
True |
PROGRAMNAME |
specObj-dr17 |
1 |
A |
z_noqso |
None |
Best redshift when ignoring QSO fits, recommended for BOSS CMASS and LOWZ targets; calculated only for survey=boss spectra, not for any SDSS spectrograph data |
False |
True |
Z_NOQSO |
specObj-dr17 |
1 |
C |
redshift_warning |
None |
Bitmask with warning on redshift result |
False |
True |
ZWARNING |
spZbest |
1 |
C |
exptime |
second |
Exposure time in seconds |
False |
True |
EXPTIME |
spPlate |
0 |
C |
extra_files |
None |
Additional files read for ingest |
False |
False |
N/A |
N/A |
N/A |
C |
ra |
deg |
Right Ascension in degrees |
True |
True |
PLUG_RA |
spZbest |
1 |
C |
file |
None |
File used for this record |
False |
False |
N/A |
N/A |
N/A |
C |
specid |
None |
Dataset-specific spectrum identifier (may not be unique) |
True |
True |
SPECOBJID |
specObj-dr17 |
1 |
C |
wavemax |
AA |
Maximum value of wavelength coverage in Angstroms |
False |
True |
WAVEMAX |
spZbest |
1 |
C |
dateobs_center |
None |
Central value of the dateobs range |
False |
True |
DATE-OBS |
spPlate |
0 |
C |
dec |
deg |
Declination in degrees |
True |
True |
PLUG_DEC |
spZbest |
1 |
C |
data_release |
None |
[Categorical] Data release of a given record (with a common data structure, e.g., SDSS-DR16, BOSS-DR16) |
False |
True |
N/A |
N/A |
N/A |
C |
spectype |
None |
[Categorical] Spectral type of the object (STAR, GALAXY, QSO) |
False |
True |
CLASS |
spZbest |
1 |
C |
site |
None |
[Categorical] Site of observations |
False |
True |
N/A |
N/A |
N/A |
C |
telescope |
None |
[Categorical] Telescope used for the observation |
False |
True |
N/A |
N/A |
N/A |
C |
specprimary |
None |
Whether an entry is the primary spectrum for a given target object |
False |
True |
SPECPRIMARY |
specObj-dr17 |
1 |
C |
datasetgroup |
None |
[Categorical] Common name for a coherent set of spectra published as a single release (e.g., SDSS_BOSS) |
False |
True |
N/A |
N/A |
N/A |
C |
targetid |
None |
Dataset-specific photometric target identifier |
False |
True |
BESTOBJID |
specObj-dr17 |
1 |
C |
updated |
None |
Date and time when the record was created/updated |
False |
False |
N/A |
N/A |
N/A |
C |
sparcl_id |
None |
Universally Unique Identifier for spectrum in SPARCL |
True |
True |
N/A |
N/A |
N/A |
C |
redshift |
None |
Measured redshift, or radial velocity in units of redshift |
False |
True |
Z |
spZbest |
1 |
C |
dateobs |
None |
Range of observational dates for a given spectrum (single value for a single date) |
False |
True |
DATE-OBS |
spPlate |
0 |
C |
wavemin |
AA |
Minimum value of wavelength coverage in Angstroms |
False |
True |
WAVEMIN |
spZbest |
1 |
C |
instrument |
None |
[Categorical] Instrument used for observation |
False |
True |
N/A |
N/A |
N/A |
C |
redshift_err |
None |
Uncertainty on the measured redshift, or radial velocity in units of redshift |
False |
True |
Z_ERR |
spZbest |
1 |
S |
mask |
None |
and_mask |
False |
True |
N/A |
spPlate |
2 |
S |
sky |
1e-17 erg cm-2 s-1 AA-1 |
Subtracted sky flux |
False |
True |
N/A |
spPlate |
6 |
S |
model |
1e-17 erg cm-2 s-1 AA-1 |
Pipeline best model fit used for classification and redshift |
False |
True |
N/A |
spZbest |
2 |
S |
ivar |
1e+34 cm4 s2 AA2 erg-2 |
Inverse variance of flux |
False |
True |
N/A |
spPlate |
1 |
S |
wave_sigma |
pixel |
Line-spread function width (sigma of approximating Gaussian) in units of number of pixel |
False |
True |
N/A |
spPlate |
4 |
S |
flux |
1e-17 erg cm-2 s-1 AA-1 |
Coadded calibrated flux |
True |
True |
N/A |
spPlate |
0 |
S |
wavelength |
AA |
Wavelength in units of Angstroms |
True |
True |
CRVAL1, COEFF1 |
spPlate |
0 |